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Stellar Birth Radii in the LMC: Insights into Chemodynamics, Radial Migration, and Star Formation across the Disk

  • Authors: Yuxi(Lucy) Lu, Bethany Garver, David L. Nidever, Joshua T. Povick, Nicolás Garavito-Camargo, Maria-Rosa L. Cioni, Danny Horta

Yuxi(Lucy) Lu et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

Histogram of the true birth radii from the simulated LMC versus the inferred birth radii using the method described in Section 2.3, colored by the number of stars (top) and the median age (bottom). We are able to successfully infer birth radii with a bias of −0.6 kpc and a RMSE of 1.5 kpc for stars <6 Gyr.

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